Introduction of Space Exploration Progress for Planetary Radio Burst Emission

PING Jinsong1,2, WANG Mingyuan1,2, ZHANG Mo1,2, CHEN Linjie1,2, DONG Liang2,3, WU Yuxiang1,2

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Journal of Deep Space Exploration ›› 2021, Vol. 8 ›› Issue (1) : 80-91. DOI: 10.15982/j.issn.2096-9287.2021.20200016
Article
Article

Introduction of Space Exploration Progress for Planetary Radio Burst Emission

  • PING Jinsong1,2, WANG Mingyuan1,2, ZHANG Mo1,2, CHEN Linjie1,2, DONG Liang2,3, WU Yuxiang1,2
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Abstract

At low frequency electron-magnetic wave band, planetary bodies not only emit thermal radiation, but also emit non-thermal radiation burst. The typical emission is planetary auroral radio burst consists of planetary kilometric wave burst, Jovian radiation at hectometer and decameter wavelengths. This kind of burst has been observed on the ground and in the space for dozens of years. The developed method can also be used as remote sensing tool to detect the inner structure of Jovian magnetosphere. However, the characteristics and mechanism have not been fully understood for the solar system planetary radio burst, there are still quite a lot of open questions left. Similar radio burst may also be observed from the exoplanetary systems. Following the development of space technology, radio astronomical observation has extended to kilometer wave. In the future the large radio array at low frequency can play key role to uncover the mechanism for the planetary radio burst, and also can be used to detect the exoplanets. The Chang’e-4 lunar mission with its low frequency payloads is working as pathfinder for the Earth Auroral Kilometer Radiation (AKR) and Jovian bursts,

Keywords

planet / radio burst / aurora / Earth / Jupiter

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PING Jinsong, WANG Mingyuan, ZHANG Mo, CHEN Linjie, DONG Liang, WU Yuxiang. Introduction of Space Exploration Progress for Planetary Radio Burst Emission. Journal of Deep Space Exploration, 2021, 8(1): 80‒91 https://doi.org/10.15982/j.issn.2096-9287.2021.20200016

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